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Hudson Alexander Loughlin - posted 10:10, Thursday 27 July 2023 - last comment - 12:19, Thursday 27 July 2023(11255)
CMTF Optical Cavity Properties
We're preparing to set up a Pound-Drever-Hall lock to lock a Mephisto laser to a stable, indium optical cavity. The cavity has mirrors labeled "Y1-1037-0-0.50cc" and "PR1-1064-99-IF-1037-UV" the Y1 mirror looks to be a high-reflector with a zero-degrees angle-of-incidence and a 0.5 meter radius of curvature. The PR1 mirror looks to be a flat mirror coated to be 99% reflective at 1064nm on a 1037-UV substrate. Based on these parameters, we expect the cavity to have a finesse of F = -2*Pi/ln(R1*R2) = 625 where R1 = 1.00 and R2 = 0.99. The spacing between the mirrors is approximately 255mm and the mirror radii of curvature are r1 = 500mm and r2 = infinity so the cavity stability factor is g = (1 - L/r1)*(1 - L/r2) = (1 - 255/500)*1 = 0.49 so the cavity has a large stability margin. (Cavities are stable as long as 0 < g < 1 and are unstable otherwise.)
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Hudson Alexander Loughlin - 12:19, Thursday 27 July 2023 (11257)GQuEST
Since the cavity mode needs to match the radius of curvature at each mirror, we can use the fact that the cavity mode has a waist at the flat mirror and a radius of curvature 1/R(z) = z/(z^2 + zR^2) to calculate the Rayleigh range zR. The waist size is related to the Rayleigh range by zR = pi*w0^2/lambda where lambda = 1064nm is the optical wavelength. Going through the math, we find that the cavity has a waist size of 291um located at its flat, partially transmissive mirror.
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